Standing Alfvén waves with m ≫ 1 in an axisymmetric magnetosphere excited by a non-stationary source

As a continuation of our earlier paper, we consider here the case of the excitation of standing Alfvén waves by a source of the type of sudden impulse. It is shown that, following excitation by such a source, a given magnetic shell will exhibit oscillations with a variable frequency which increa...

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Main Authors: A. S. Leonovich, V. A. Mazur
Format: Article
Language:English
Published: Copernicus Publications 1998-08-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/16/914/1998/angeo-16-914-1998.pdf
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author A. S. Leonovich
V. A. Mazur
author_facet A. S. Leonovich
V. A. Mazur
author_sort A. S. Leonovich
collection DOAJ
description As a continuation of our earlier paper, we consider here the case of the excitation of standing Alfvén waves by a source of the type of sudden impulse. It is shown that, following excitation by such a source, a given magnetic shell will exhibit oscillations with a variable frequency which increases from the shell's poloidal to toroidal frequency. Simultaneously, the oscillations will also switch over from poloidally (radially) to toroidally (azimuthally) polarized. With a reasonably large attenuation, only the start of this process, the stage of poloidal oscillations, will be observed in the ionosphere.<br><br><b>Key words.</b> Ionosphere-magnetosphere interactions · Wave propagation · MHD waves and instabilities</p>
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spelling doaj.art-129b815fe51d439b95764ebed9e4ec692022-12-21T18:44:34ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05761998-08-011691492010.1007/s00585-998-0914-zStanding Alfvén waves with m &#x226B; 1 in an axisymmetric magnetosphere excited by a non-stationary sourceA. S. Leonovich0V. A. Mazur1Institute of Solar-Terrestrial Physics (ISTP), Russian Academy of Science, Siberian Branch, Irkutsk 33 P.O.Box 4026, 664033 Russia e- mail: leon@iszf.irk.ruInstitute of Solar-Terrestrial Physics (ISTP), Russian Academy of Science, Siberian Branch, Irkutsk 33 P.O.Box 4026, 664033 Russia e- mail: leon@iszf.irk.ruAs a continuation of our earlier paper, we consider here the case of the excitation of standing Alfvén waves by a source of the type of sudden impulse. It is shown that, following excitation by such a source, a given magnetic shell will exhibit oscillations with a variable frequency which increases from the shell's poloidal to toroidal frequency. Simultaneously, the oscillations will also switch over from poloidally (radially) to toroidally (azimuthally) polarized. With a reasonably large attenuation, only the start of this process, the stage of poloidal oscillations, will be observed in the ionosphere.<br><br><b>Key words.</b> Ionosphere-magnetosphere interactions · Wave propagation · MHD waves and instabilities</p>https://www.ann-geophys.net/16/914/1998/angeo-16-914-1998.pdf
spellingShingle A. S. Leonovich
V. A. Mazur
Standing Alfvén waves with m &#x226B; 1 in an axisymmetric magnetosphere excited by a non-stationary source
Annales Geophysicae
title Standing Alfvén waves with m &#x226B; 1 in an axisymmetric magnetosphere excited by a non-stationary source
title_full Standing Alfvén waves with m &#x226B; 1 in an axisymmetric magnetosphere excited by a non-stationary source
title_fullStr Standing Alfvén waves with m &#x226B; 1 in an axisymmetric magnetosphere excited by a non-stationary source
title_full_unstemmed Standing Alfvén waves with m &#x226B; 1 in an axisymmetric magnetosphere excited by a non-stationary source
title_short Standing Alfvén waves with m &#x226B; 1 in an axisymmetric magnetosphere excited by a non-stationary source
title_sort standing alfven waves with m x226b 1 in an axisymmetric magnetosphere excited by a non stationary source
url https://www.ann-geophys.net/16/914/1998/angeo-16-914-1998.pdf
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